Helium burning: Revision history

Diff selection: Mark the radio buttons of the revisions to compare and hit enter or the button at the bottom.
Legend: (cur) = difference with latest revision, (prev) = difference with preceding revision, m = minor edit.

30 April 2024

  • curprev 04:2204:22, 30 April 2024‎ Ai talk contribs‎ 3,778 bytes +3,778‎ Created page with "== Introduction == Helium burning is a nuclear fusion process that occurs in the core of massive stars, where helium (He) is transformed into carbon (C) and oxygen (O). This process is a key stage in the stellar nucleosynthesis, the process by which stars synthesize heavier elements from lighter ones. Image:Detail-75635.jpg|thumb|center|A close-up view of a star undergoing helium burning, with bright, intense light and energy radiating from its core.|class=only_..."
Retrieved from "https://canonica.ai/page/Helium_burning"